Triple

T19730175
Position Surface form Disambiguated ID Type / Status
Subject Messier 4 E473829 entity
Predicate hasNotableObject P5510 FINISHED
Object PSR B1620−26 — NE NERFINISHED

How this triple was built (3 steps)

Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.

NER Named-entity recognition gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: PSR B1620−26 | Statement: [Messier 4, hasNotableObject, PSR B1620−26]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07 
Target entity: PSR B1620−26
Context triple: [Messier 4, hasNotableObject, PSR B1620−26]
  • A. PSR B0531+21
    PSR B0531+21 is the highly magnetized, rapidly rotating neutron star at the center of the Crab Nebula, serving as one of the most studied pulsars in astrophysics.
  • B. Cygnus X-2
    Cygnus X-2 is a bright low-mass X-ray binary system in the constellation Cygnus, consisting of a neutron star accreting matter from a companion star and serving as an important source for studying X-ray emission and compact objects.
  • C. Scorpius X-1
    Scorpius X-1 is a bright low-mass X-ray binary system and one of the strongest persistent X-ray sources in the sky, located in the constellation Scorpius.
  • D. Cygnus X-1
    Cygnus X-1 is one of the strongest known X-ray sources in the sky and the first widely accepted stellar-mass black hole candidate, located in the constellation Cygnus.
  • E. Holmberg II X-1
    Holmberg II X-1 is an ultraluminous X-ray source in the dwarf galaxy Holmberg II, believed to be powered by accretion onto a compact object such as a black hole.
  • F. None of above. chosen
  • G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2 Entity disambiguation (via description) gpt-5-mini-2025-08-07 
Target entity: PSR B1620−26
Target entity description: PSR B1620−26 is a millisecond pulsar in the globular cluster Messier 4, notable for hosting a circumbinary planet in a triple system with a white dwarf companion.
  • A. PSR B0531+21
    PSR B0531+21 is the highly magnetized, rapidly rotating neutron star at the center of the Crab Nebula, serving as one of the most studied pulsars in astrophysics.
  • B. Cygnus X-2
    Cygnus X-2 is a bright low-mass X-ray binary system in the constellation Cygnus, consisting of a neutron star accreting matter from a companion star and serving as an important source for studying X-ray emission and compact objects.
  • C. Scorpius X-1
    Scorpius X-1 is a bright low-mass X-ray binary system and one of the strongest persistent X-ray sources in the sky, located in the constellation Scorpius.
  • D. Cygnus X-1
    Cygnus X-1 is one of the strongest known X-ray sources in the sky and the first widely accepted stellar-mass black hole candidate, located in the constellation Cygnus.
  • E. Holmberg II X-1
    Holmberg II X-1 is an ultraluminous X-ray source in the dwarf galaxy Holmberg II, believed to be powered by accretion onto a compact object such as a black hole.
  • F. None of above. chosen

Provenance (2 batches)

The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.

Step Stage Batch ID Status When
creating Elicitation batch_69d8e517ebd48190979ee76723bcfadf completed April 10, 2026, 11:55 a.m.
NER Named-entity recognition batch_69e649fbeaf081909e9356229eaf84dd completed April 20, 2026, 3:45 p.m.
Created at: April 10, 2026, 1:47 p.m.